CWNU 3592

0.20 UTI

0.0

C_N

0.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 22

Radius (P>50% members) 2.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.0 Very loose
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 3592 is a sparse, very loose object of very high C3 quality. Its parallax locates it at a very large^* distance, well below the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~153.85 kpc) differs significantly from the median photometric distance (~13.49 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Extremely distant High extinction Very young

Data

🔍 Search references for CWNU 3592 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	242.565	-54.979	0.006	-2.883	-2.959	–
He et al.	2023	242.565	-54.978	0.005	-2.871	-2.959	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
He et al.	2023	13.49	3.20	–	2	–	–	–	–

Visualization

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